Frame of Reference is a precision cinematography platform for working DPs, ACs, and film students. Dictionary, calculators, testing tools, and industry resources — all in one place.
EST. MMXXVI · LOS ANGELES
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Film Dictionary
Searchable glossary of cinematography terms, lens vocabulary, lighting concepts, and crew positions with categories.
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Photometrics
Calculate T-stops from foot-candles and ISO. Inverse square law fall-off. Lux and foot-candle conversions.
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Over / Under
Generate exposure latitude test charts with customizable stop range and increments — ⅓, ½, or full stops.
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Resources
Mentorship and fellowship opportunities, unions and societies, and essential apps for working cinematographers.
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The Gallery
Behind the scenes photography from film sets — lighting rigs, camera setups, crew at work, and the world behind the lens.
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Database
Searchable specs for cinema cameras, lenses, and lighting fixtures — tungsten and LED — with native ISOs, dynamic range, formats, and output data.
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// 02 — REFERENCE
Film Dictionary
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// Category
// 03 — TOOLS
Photometrics Calculator
// 01 — What is Photometrics?
Light is just math.
Photometrics is the science of measuring light. As a cinematographer, it gives you a precise, repeatable language for light — so instead of guessing whether your key light is bright enough, you can measure it, calculate your exposure, and know exactly what T-stop to set before you even roll camera.
There are three numbers you work with constantly:
fc
Foot-Candles
How much light is hitting your subject. Measured with a light meter. 1 fc = 10.76 lux.
ISO
Sensitivity
How sensitive your camera sensor (or film) is to light. Higher ISO = more sensitive = less light needed.
T
T-Stop
The aperture setting on your lens. The result of your calculation — this is what you dial in.
// 02 — The Inverse Square Law
Move a light twice as far — get four times less light.
This is the single most important rule in cinematography lighting. The Inverse Square Law states: when you double the distance between a light and your subject, the intensity drops to one quarter — not one half.
It feels counterintuitive at first. But think of it this way: light spreads out in all directions as it travels. When it has to cover twice the distance, it has to cover four times the area. So the same amount of light is now spread over four times as much space.
// Inverse Square Law — Light Spread Diagram
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The Rule: Double the distance → ¼ the light. Halve the distance → 4× the light. This is why moving a light even a foot or two makes a dramatic difference up close, but almost none when it's already far away.
// 03 — Practical Examples
Three real-world scenarios.
01
Interior Interview — Single Key Light
You're lighting a talking head interview. Your ARRI SkyPanel S60 is 8 feet from your subject. Your light meter reads 160 foot-candles at the subject. You're shooting at ISO 800, 180° shutter, 24fps.
Exposure time (180° @ 24fps)1/48 sec = 0.0208s
T-Stop = √(fc × t × ISO ÷ 250)= √(160 × 0.0208 × 800 ÷ 250)
ResultT2.8 — a wide, shallow aperture ✓
02
Moving the Light — Inverse Square Law in Action
Same setup. The director asks you to push the light back to 16 feet — double the original distance. What happens to your exposure?
New intensity160 × (8÷16)² = 160 × 0.25 = 40 fc
New T-stop (same ISO)T1.4 — nearly wide open
To maintain T2.8Raise ISO from 800 → 3200
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Doubling the distance costs you 2 full stops. This is why cinematographers keep lights close when they want a specific look — and why moving a light just 2 feet closer to a subject can dramatically change the feel of a shot.
03
Night Exterior — Finding Your Exposure
You're on a night exterior. Your 4K HMI is positioned 20 feet from your subject. Meter reads 64 foot-candles. You want to shoot at T4 for depth of field. What ISO do you need?
Target T-stopT4 (want depth of field)
Formula rearranged for ISOISO = (T² × 250) ÷ (fc × t)
= (16 × 250) ÷ (64 × 0.0208)= 4000 ÷ 1.33
ResultISO ≈ 800 — clean, no noise ✓
04
Lux vs Foot-Candles — Working Internationally
You're on a European production. The gaffer hands you a meter reading in lux — the international standard. Your meter reads 1,076 lux. What's that in foot-candles, and what T-stop does that give you?
Convert: lux ÷ 10.7641076 ÷ 10.764 = 100 fc
T-Stop at ISO 400, 180° / 24fps= √(100 × 0.0208 × 400 ÷ 250)
ResultT2.0 — a fast, shallow look ✓
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Remember: 1 foot-candle = 10.764 lux. American productions use foot-candles. The rest of the world uses lux. Your light meter will have a switch — always confirm which unit it's displaying before calculating.
// 04 — Quick Reference
The three rules to remember.
÷4
Double = Quarter
Double the distance from subject, lose 2 stops of light. The inverse square law.
fc×lux
Convert Units
fc → lux: multiply by 10.764. lux → fc: divide by 10.764.
T=√
The Formula
T = √(fc × exposure time × ISO ÷ 250)
T-Stop Calculator
Calculate the required T-stop from incident light reading and ISO.
T-Stop—T
Exposure Time—sec
EV—
Light Fall-Off
Calculate new intensity at a different distance using the inverse square law.
New Intensity—fc
Ratio—×
Stop Difference—stops
Lux / Foot-Candle Converter
Convert between lux and foot-candles. 1 fc = 10.764 lux.
Foot-Candles → Lux—lx
Lux → Foot-Candles—fc
// 04 — TOOLS
Over / Under Calculator
// 01 — Dynamic Range & Latitude
How much light can your camera see?
Every camera — film or digital — can only record a limited range of brightness at once. Too bright and detail disappears into white. Too dark and it disappears into black. Dynamic range is the total distance between those two points, measured in stops.
A stop is a doubling or halving of light. Your eye can see roughly 20 stops of dynamic range. A consumer camera might see 8–10. A professional digital cinema camera like the ARRI ALEXA 35 sees up to 17 stops. 35mm film sits around 13–14 stops, but handles the extremes very differently than digital.
// Dynamic Range — Stops of Latitude
Latitude is how forgiving that range is. It's how many stops over or under the "correct" exposure you can push before the image falls apart. A camera with wide latitude means you can recover badly exposed footage in post. A camera with narrow latitude means you have to nail the exposure on set.
8–10
Consumer Camera
Typical DSLR or mirrorless. Clips highlights fast and crushes shadows quickly.
13–14
35mm Film
Narrower than top digital, but with a beautiful, gradual rolloff in highlights and shadows.
14–17
Cinema Digital
ARRI, RED, Sony VENICE class. Wide latitude with Log encoding to preserve detail.
// 02 — Over / Under Testing
Testing tells you exactly where your camera breaks.
An over/under test — also called an exposure latitude test — is how cinematographers map a camera's usable range before they shoot. You photograph the same scene at a series of stops above and below your base exposure, then evaluate the footage in a controlled color suite.
You're answering three questions:
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Highlight Latitude
How many stops over base exposure before highlights clip with no recovery? Where does the rolloff begin?
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Shadow Latitude
How many stops under before shadows crush to black with visible noise? Can details be lifted in post?
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Noise Character
At which stop does noise become unacceptable? Is it fine grain or color noise? How does ISO affect it?
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Cinematographers run these tests before every major production. The results inform everything from how you expose on set (ETTR vs protecting shadows) to how your colorist knows what they can pull back in the grade.
// 03 — The Toe & The Knee
How film handles the edges of exposure.
35mm film doesn't clip highlights the way digital does. Instead, it has an S-curve response — a gradual, elegant rolloff at both the dark and bright extremes. This curve has two named regions.
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The Toe — the bottom of the curve, in the shadows. Film's toe means dark areas don't crush to pure black immediately — they roll off gently, preserving shadow detail with a characteristic "lift" that photographers call shadow density. It's one of the reasons film feels so rich in dark scenes.
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The Knee — the top of the curve, in the highlights. Film's knee is where exposure compression begins. Highlights don't blow out with a hard edge — they compress and shoulder off gradually, giving skin tones and skies a soft, retained quality even when overexposed.
// Film H&D Curve vs Digital Response
How this relates to digital cinematography: Modern digital cinema cameras use Log gamma curves to mimic the S-curve behavior of film. But what exactly is a Log curve — and why does it matter?
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The simplest way to think about Log:
Imagine your camera can record 14 stops of light — from deep black to pure white. Now imagine you have to fit all 14 stops into a box with only 1,024 slots (the values your codec can store).
Without Log (linear recording): the camera spreads those 1,024 slots evenly. Your shadows get a tiny slice and your highlights get most of the space — but your eye sees shadows as the most important part of the image. You end up with noisy blacks and clipped highlights.
With Log: the camera uses math to squeeze the bright stuff together (giving it fewer slots) and spread the dark stuff out (giving it more slots). The image looks flat and washed out on a monitor — but all the information is still there, packed efficiently. A colorist can then "open it up" in post and get a full, rich, detailed image out of it.
// Log vs Linear — How Values Are Distributed
// What Log Looks Like — Before & After Grade
FLAT
Looks Wrong On Set
Log footage looks grey and washed out. That's normal. Use a monitoring LUT on set to preview how the final grade will look.
INFO
Packs In Data
The flat look means the codec is recording as much information as possible — all your highlight and shadow detail is still there.
GRADE
Built For Post
Log footage is designed to be transformed by a colorist. The grade "unpacks" the data into a rich, contrasty final image.
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Common Log formats: ARRI LogC (ALEXA cameras), Sony S-Log3 (VENICE, FX9), Canon Log 3 (C70, C300), RED Log3G10 (DSMC2/3). Each is slightly different — but they all do the same job: pack the maximum information into the file for the colorist to work with.
But there's a key difference from film: digital clips hard. When film blows out, it rolls off gracefully to white. When digital clips, it's a sharp mathematical wall — detail goes to 100% white and stays there. Log helps you get close to the edges, but it doesn't change what happens past them.
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The practical takeaway: Film's latitude was forgiving because of its natural S-curve. With digital, you have more total stops — but they're distributed differently. An over/under test maps exactly where your digital camera's "shoulder" begins so you can expose like a film shooter: protect the highlights, and lift the shadows in post.
// 04 — Practical Examples
Three real-world scenarios.
01
The Window Scene — Protecting Highlights
A character sits near a bright window. The DP exposes for the face. Later in the DI suite, the colorist pulls the test frames and discovers the window blows out at +3 stops above base on the ALEXA 35 — but starts compressing at +2. The DP knows: expose with the face at -1 stop from base, giving +3 stops of headroom before hard clipping. The window detail is recoverable.
Test findingHard clip at +3 stops above base
Knee begins+2 stops — compression starts here
DP decisionExpose face -1 stop, window retains detail
02
Night Alley — Mapping Shadow Latitude
The DP is shooting a night exterior. They need deep blacks but also want to recover ambient detail in the alleys. An over/under test at ISO 800 and ISO 3200 (the camera's second base ISO) reveals that at ISO 800, usable shadow detail runs to -4 stops before noise takes over. At ISO 3200, noise arrives at -2 stops but highlights hold more gracefully.
ISO 800 shadow floor-4 stops from base
ISO 3200 shadow floor-2 stops — noisier sooner
DP decisionShoot ISO 800 — lift alleys in grade
03
Film vs Digital — The Rolloff Difference
A DP shooting on Kodak Vision3 500T and digitizing on a film scanner compares the shoulder rolloff to footage shot on a RED MONSTRO in the same location. Both cameras have similar total stops, but the film's highlights hold texture two full stops longer before going to white — the knee is far more graceful. This is why DPs and colorists add a "film emulation" S-curve to digital footage in post.
Film highlight rolloffGradual over 2+ stops — retains texture
Digital highlight rolloffHard clip — zero-to-white in under a stop
In practiceProtect digital highlights. Pull back in grade.
04
Reading the Test — What to Look For
After running your over/under test, bring all frames into DaVinci Resolve with no grade applied (pure Log). Lay them on the timeline in order from most underexposed to most overexposed. Check a waveform monitor and evaluate each frame at the same position.
-4 to -5 stopsWhere does noise become distracting?
-1 to -3 stopsHow much shadow detail lifts cleanly?
BASEReference. Should match your meter reading.
+1 to +2 stopsWhere does the highlight knee begin?
+3 to +5 stopsWhere does it go to pure white with no recovery?
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Use the Over/Under Calculator on this page to generate your test chart, then log your findings in the Testing section (page 08) to build a permanent record of every camera you shoot on.
// 05 — Summary
What every DP needs to know.
D.R.
Know Your Range
Test every camera before the shoot. Latitude varies by ISO, firmware, and shooting mode.
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Protect Highlights
Digital clips hard at the top. Film rolls off. Keep your exposure just below the knee.
Log
Shoot Log
Log gamma mimics the film S-curve. It preserves the most information for the colorist to work with.
// ND Filter Stack
No ND filters added. Click + Add ND to stack filters.
Total ND StackND 0.0= 0 stops
Stop
ISO / EI
Shutter
T-Stop
ND Filter
Relative Exposure
◈ Over/Under testing evaluates your camera's exposure latitude. Each row represents one test frame. Expose at the indicated value relative to your base, then review in DI to assess highlight and shadow retention.
// 09 — DATABASE
Equipment Database
// Category
// Cinema Cameras
Camera Specs
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Camera
Sensor
Res.
Native ISO
Dyn. Range
Format
// Film Stocks
Film Stocks
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// Cinema Lenses
Lens Specs
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Lens
Type
Coverage
T-Stop Range
Close Focus
Format
// Lighting Fixtures
Lighting Database
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Fixture
Power
Color Temp
Output
Beam Angle
CRI
Notes
// Screenplays
Screenplay Library
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// Plans & Pricing
Choose Your Plan
Professional tools. Accessible pricing.
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✓ Full cinematography dictionary (80+ terms)
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✓ Over/Under chart generator
✓ Full equipment database — cameras, lenses, lights
✓ Screenplay library
✓ Industry resources & podcasts
✓ The Gallery
○Saved terms library
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○ND filter stack
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// Tier 02
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// Tier 03
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// 05 — LIBRARY
Saved Library
// 08 — TESTING
Camera Testing
// Category
// Camera — Over / Under
Exposure Latitude Testing
// Saved Tests
Test NameSaved ✓
Stop
ISO / EI
Shutter
T-Stop
Relative Exposure
// Camera — Lens Testing
Lens Test Sheet
Fill in the specs for each lens tested. Add a new row per lens or per focal length setup.
Lens Test Log
Saved ✓
#
Camera
Format
Shooting Mode
Codec
Resolution
Color Temp
Native ISO
Lens Type
Focal Length
Anamorphic
Spherical
Zoom
// Lighting Testing
Lighting Test Log
Record lighting setups, fixture performance, modifier tests, and photometric readings for each fixture tested.
Lighting Test Log
Saved ✓
#
Fixture
Manufacturer
Wattage / Power
Color Temp (K)
Distance (ft)
Reading (fc)
Modifier
CRI / TLCI
Notes
// 06 — RESOURCES
Industry Resources
// Category
// 01 — Mentorship
Mentorship Opportunities
Programs connecting emerging cinematographers with experienced DPs and industry professionals for career guidance and development.
AFI Conservatory Mentorship
American Film Institute pairs emerging cinematographers with established DPs for guided career development and project feedback.
Founded by acclaimed DP Natasha Braier ADF ASC, Deep-Light is a mentorship program dedicated to supporting emerging cinematographers — particularly those from underrepresented backgrounds — through direct guidance, industry access, and creative development.
Issa Rae's initiative supporting writers and directors of color in television and film, providing mentorship, development resources, and access to industry networks.
Film Independent's signature diversity fellowship connecting emerging filmmakers from underrepresented communities with mentors, resources, and a collaborative feature film production.
The American Society of Cinematographers' podcast featuring in-depth conversations with ASC members on projects, philosophy, and the state of the craft.
John August and Craig Mazin's long-running screenwriting podcast — essential listening for understanding story structure, a core skill for any visual storyteller.
Roger and James Deakins discuss cinematography, filmmaking, and visual storytelling with guests — a rare window into the mind of a two-time Oscar-winning DP.
Tools, databases, and platforms for building mood boards, referencing shot compositions, and exploring the visual language of cinema.
Shot Deck
The world's largest searchable database of film stills, organized by cinematographer, director, film, color palette, lens, and composition type. An essential reference tool for any DP in prep.
AI-powered visual reference and mood board tool for filmmakers. Generate lighting diagrams, color references, and stylistic lookbooks tailored to your project's visual direction.
Widely used by DPs and directors, Notion offers customizable templates for organizing visual references, look development notes, and production design boards.
The British Film Institute's streaming platform offering access to classic and international cinema — an invaluable resource for studying visual storytelling and cinematographic technique.
A landmark video essay series by Tony Zhou and Taylor Ramos analyzing visual style, composition, and cinematic language across film history. Essential viewing for cinematographers.
The gold standard of curated cinema — a streaming library of landmark films with supplements, essays, and context. Essential for building a visual vocabulary grounded in film history.
Adobe's color palette tool allows cinematographers to extract palettes from reference images, explore complementary color schemes, and share color stories with production design teams.